most citedThe eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection

38 citations · 96 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20178 cited

Observation of a Large-scale Quasi-circular Secondary Ribbon associated with Successive Flares and a Halo CME

Eun-Kyung Lim, Vasyl Yurchyshyn, Pankaj Kumar +7

Solar flare ribbons provide an important clue to the magnetic reconnection process and associated magnetic field topology in the solar corona. We detected a large-scale secondary f…

astro-ph.SR201718 cited

Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped Flare

Chaowei Jiang, Xiaoli Yan, Xueshang Feng +4

As a fundamental magnetic structure in the solar corona, electric current sheets (CSs) can form either prior to or during solar flare, and they are essential for magnetic energy di…

astro-ph.SR201738 cited

The eruption of a small-scale emerging flux rope as the driver of an M-class flare and a coronal mass ejection

X. L. Yan, C. W. Jiang, Z. K. Xue +6

Solar flares and coronal mass ejections (CMEs) are the most powerful explosions in the Sun. They are major sources of potentially destructive space weather conditions. However, the…

astro-ph.SR201725 cited

Comparison of Two Coronal Magnetic Field Models for Reconstructing a Sigmoidal Solar Active Region With Coronal Loops

Aiying Duan, Chaowei Jiang, Qiang Hu +4

Magnetic field extrapolation is an important tool to study the three-dimensional (3D) solar coronal magnetic field which is difficult to directly measure. Various analytic models a…

astro-ph.SR20177 cited

A Magnetic Bald-Patch Flare in Solar Active Region 11117

Chaowei Jiang, Xueshang Feng, S. T. Wu +1

With SDO observations and a data-constrained MHD model, we identify a confined multi-ribbon flare occurred on 2010 October 25 in solar active region 11117 as a magnetic bald patch…